Sbarufatti (INAF/OAB - IASF Pa) report on behalf of the Swift-XRT team: We have analysed 4. , GCN Circ. Page (U. , GCN Circ. Lien (GSFC/UMBC) and B. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. GCN Circ. La Parola (INAF-IASF Pa), T. Barthelmy (GSFC), V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. it> B. Here’s how you knowDOI: 10. it> B. I am an astrophysicist. Boris Sbarufatti at INAF-OAB/IASFPA <boris. In extremely urgent cases, after trying the Burst Advocate, you can contact the. inaf. (Feb 11, 2013) Published in: Astron. it> B. P. Leicester), A. 5 hours after the trigger. Guidorzi (INAF OAB) and D. L. 10983), from 68 s to 58. Sbarufatti (INAF-OAB/IASFPA), R. Content may be subject to copyright. inaf. Sbarufatti (PSU), K. (GCN Circ. Melandri (INAF-OAB) and B. Kennea (PSU), A. These topic labels come from the works of this person. P. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 13:37:25 UT, the Swift Burst Alert Telescope (BAT) detected a peak in an image at a location near to the known. Sbarufatti, V. Markwardt and Span and David M. 7 ks after the BAT trigger. Pascoli, I-06123 Perugia, Italy 2. Krimm (GSFC/USRA), M. Sbarufatti (PSU) report on behalf of. La Parola, B. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status. it> S. GCN Circ. A. J. it> B. Sakamoto (AGU) and B. csv file deleting the 1st line) but nothing (steps, sleep, etc. Amaral-Rogers (U. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Evans (U. The sample has a high level of completeness in redshift (90%). P. P. We have analyzed 14. R. Boris Sbarufatti at PSU <bxs60@psu. inaf. La Parola, [email protected]° decl: 59. 2 ks to 383. P. (2008). Burst Advocate for this burst is B. Sbarufatti (INAF OAB/INAF IASF-PA) , V. , GCN Circ. Y. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. 10979), from 82 s to [email protected]. 7685) in Window Timing mode, 146 s after the BAT trigger. Copy reference. Sbarufatti (INAF-OAB/IASFPA), V. P. Siegel (PSU) report on behalf of the Swift team. sbarufatti@brera. Krimm (NSF), N. Sbarufatti (INAF-OAB/PSU), P. Physics Department University of Perugia, and I. This page has only limited features, please log in for full [email protected] Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. inaf. 345 was measured for. Sbarufatti (INAF-OAB/IASFPA), J. NASA’s Swift satellite recently detected a rising tide of high-energy X-rays from a source toward the center of our Milky Way galaxy. 4 ks, with a 1. inaf. Sbarufatti B. Leicester), A. Holland (GSFC/USRA), H. Cummings (NASA/UMBC) report on behalf of the Swift-XRT team The XRT began observing the field of GRB 090531B (trigger 353728, Cummins, et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Kennea (PSU), B. A. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Osborne (U. it> B. ) has clearly shown that the host galaxies are massive and luminous ellipticals. it). 8 ks after the BAT trigger. 3 ks of XRT data for GRB 100725A (Markwardt et al. D'Avanzo (INAF-OAB), V. csv file with my fitbit activities for the past month. H. A. 9603) on 2009 July 2 at 14:15 UT, 3. inaf. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Leicester) and D. GCN Circ. . It is not an astrophysical event. De Pasquale (MSSL) report on behalf of the Swift Team. inaf. L. 2 ks of XRT data for GRB 130725B (Swenson et al. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Fariborz Besarati (born 23 August 1966) is a Swedish former wrestler who competed in the 1992 Summer Olympics and in the 1996 Summer Olympics. it> B. GCN Circ. Sbarufatti (PSU), A. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 13:37:25 UT, the Swift Burst Alert Telescope (BAT) detected a peak in an image at a location near to the known. 0 ks to 196. sbarufatti@brera. Sbarufatti, V. 4-3658}, author={Craig B. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone. Barun was a naughty child. sbarufatti@brera. (2005a, 2006). Sbarufatti over 6 years ago. it Stefano Ciprini 1. A. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. it> B. D. 21822), from 63 s to 924 s after the BAT trigger. L. , Ciprini, S. Racusin, Eleonora. La Parola, V. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. A. Sbarufatti et al. 26031), from 3. it> B. sbarufatti AT brera. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. Semantic Scholar extracted view of "GRB 150527A: Swift-XRT refined Analysis. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. In this framework, initially proposed to explain GRBs with precursor activity, the prompt emission is produced by accretion of matter onto a newly–born magnetar, and. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. , GCN Circ. 4 ks after the BAT trigger. 5 UT, 92. inaf. Holland 1,2,3, Boris Sbarufatti 4, Rongfeng Shen 5, Patricia Schady 6, Jay R. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. it> B. Sbarufatti, V. Sbarufatti (INAF-OAB/IASFPA), R. Osborne (U. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 11:10:45 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRS 1716-249/GRO J1719-24/V2293 Oph. inaf. A. The source has faded with respect to the initial. inaf. DOI: 10. Pagani (U. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. (2005b, 2006a, 2009), Paper I, II. V. Sbarufatti (INAF-OAB/PSU), H. N. Download full-text PDF Read full-text. GCN Circ. A. Sbarufatti (INAF IASF-Pa), V. Sbarufatti, V. sbarufatti@brera. edu> P. Tohuvavohu (U. sbarufatti@brera. Sbarufatti, V. edu> B. The data are all in Photon Counting (PC) mode. A. Holland (GSFC/USRA), H. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 11813 ). Holland1,2,3, Boris Sbarufatti4, Rongfeng Shens, Patricia Schady6, Jay R. Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. Evans (U. F. Holland (CRESST/USRA/GSFC) report on behalf of the Swift XRT team: We have analysed the first two orbits of XRT data of GRB 070529 (Holland et al. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. A. D'Avanzo (INAF-OAB), J. inaf. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. R. C. 29529). Y. Sbarufatti (INAF OAB/INAF IASF-PA) , V. Kennea (PSU), H. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. H. Sbarufatti, V. B. 8 ks after the BAT trigger. new redshifts, by B. Mangano, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The XRT began observations of GRB 080605 (trigger=313299, Sbarufatti et al. The source has faded with respect to the initial. The data are entirely in [email protected]. Mangano, V. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. it> V. Mangano (INAF-IASF PA) on behalf of the Swift XRT team Swift XRT started a ToO observation of the INTEGRAL burst GRB080120 at 19:47 UT. Krimm (GSFC/USRA), M. D'Ai (INAF-IASFPA), D. A. 2 ks exposure time. 9 ks to T+391. We have analyzed 14. Brett Sholtis was a health reporter for WITF/Transforming Health until early 2023. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. Boris Sbarufatti at PSU <[email protected] T. , GCN Circ. 11944), from 2. inaf. , GCN circ. Sbarufatti (PSU), A. sbarufatti@brera. H. 6560 ), consisting of 150 s in Window Timing. , GCN Circ. At the present day, spectroscopic follow up of unclassified blazars have been mainly performed with 4 m or 8 m class telescopes (e. Lien (GSFC/UMBC), A. Sbarufatti (INAF-OAB/PSU), H. 1 Similar Profiles; gamma ray bursts Physics & Astronomy 100%. La Parola (INAF-IASFPA), S. Marshall (NASA/GSFC), A. Evans (U. inaf. 9 ks of data of the ToO observation of GRB 080120, started on Jan 20 at 19:47 UT. Boris Sbarufatti at PSU <bxs60@psu. GCN Circ. GRB 090417B was an unusually long burst with a T 90 duration of at least 2130 s and a multi-peaked light curve at energies of 15-150 keV. B. Mangano (INAF IASF-PA), B. Gehrels (GSFC), S. inaf. (GCN 6891) due to the large offset between the initial BAT position and XRT position. We present the detection of persistent soft X-ray radiation with –1042 erg s–1 at the location of the. M. Boris Sbarufatti at PSU <bxs60@psu. A. Kennea (PSU), B. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. 1 ks. (GCN Circ. Boris Sbarufatti (CoI) (ESA Member) Dr. (INAF-IASFPA) report on behalf of the Swift Team: We have analysed the first six orbits of Swift-XRT data obtained from GRB 090417B (trigger 349450; Sbarufatti, et al. Boris Sbarufatti INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Via Ugo La Malfa 153, I-90146 Palermo, Italy E-mail: sbarufatti@ifc. Melandri (INAF-OAB), B. 2 ks of Photon Counting. J. 0 ks after the BAT trigger. inaf. De Pasquale (MSSL) report on behalf of the Swift Team. A. 4 ks after the BAT trigger. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. Gianpiero Tagliaferri, Ruben Salvaterra, Sergio Campana, Stefano Covino, Paolo D'Avanzo, Dino Fugazza, Giancarlo Ghirlanda, Gabriele Ghisellini, Andrea Melandri, Lara. La Parola, V. inaf. GCN Circ. (GCN Circ. 2 ks of XRT data for GRB 110106B (Sbarufatti et al. it> B. 1 Larger Context A major frontier in the study of astronomical sources is the development of multi-messenger as-tronomy (MMA). Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. 7 ks after the BAT trigger. it> B. The enhanced XRT position was given in Osborne et al. B. La Parola (INAF-IASFPA), S. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. N. Sbarufatti (PSU), A. Here’s how you knowUsing Webb’s spectacular sensitivity, scientists captured the first mid-infrared spectrum from space of a kilonova, which marked Webb’s first direct look at an individual heavy element from such an event. Lien (GSFC/UMBC) and B. , GCN Circ. M. it> B. Y. The data comprise 288 s in Windowed Timing (WT) mode (the first. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. A. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Download PDF. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Sbarufatti (boris. D'ai (INAF-IASFPA), [email protected]@brera. In extremely urgent cases, after trying the Burst Advocate,. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. it> B. L. Lien (GSFC/UMBC) and B. Sbarufatti (INAF OAB/IASF PA), V. [email protected] ks of exposure we don t detect. 11944), from 2. Hagen (PSU) report on behalf of the Swift team Swift performed a follow up observation of GRB 150418A, with a pointing in the direction of Source #1 reported by Sbarufatti et al. 4 ks after the BAT trigger. 8462) at 17:46:11. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. T. inaf. 9 ks to T+391. 3 ks of XRT data for GRB 110915A (Holland et al. inaf. The enhanced XRT position was given in Osborne et al. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. 2 ks of XRT data for GRB 110106B (Sbarufatti et [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Due to an observing constraint, Swift will not slew until T0+49. inaf. edu> B. The data comprise 1. Leicester), V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 7687). Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. inaf. Boris Sbarufatti at PSU <bxs60@psu. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. Cummings (GSFC/UMBC), N. 1811E, 25. Leicester) and K. N. Margutti (INAF-OAB), S. An extension of the sample, by B. Leicester) and P. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. 29529). The observation is in PC mode and consists of 1. Boris Sbarufatti at INAF-OAB/IASFPA <boris. From: Boris Sbarufatti [v1] Mon, 20 Oct 2008 14:06:52 UTC (133 KB) Full-text links: Download: Download a PDF of the paper titled ESO VLT optical spectroscopy of BL Lacertae objects. B. Y. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. Sbarufatti (INAF-OAB/IASFPA), J. Burrows (PSU) and P. sbarufatti@brera. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: Swift performed a second target of opportunity observation of GRB 110319B on March 23, 2011. g. Cancel;"The pattern we're seeing is observed in X-ray novae where the central object is a black hole," said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, currently working. Barthelmy (GSFC), P. Barthelmy (GSFC), P. Laha (GSFC/UMBC/CRESST) and B. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. inaf. 29529). GCN Circ. D'Avanzo (INAF-OAB) and P. ///// TITLE: GCN CIRCULAR NUMBER: 5856 SUBJECT: GRB 061126: Swift/UVOT Afterglow Detection DATE: 06/11/26 09:53:47 GMT FROM: Daniel E. Of the two unknown sources reported by. 9 ks after the Swift/BAT trigger. T. Mangano (INAF/IASF_PA) and C. Roma-BZCA T blazars in the P alermo BA T Survey B. 270 UTC: ra: 86. 2006) it remains one of the f ew bright sour ces. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Mangano (INAF-IASF Pa) report on behalf of the Swift-XRT team: Swift began observing the field of the Swift BAT Slew Survey (BATSS) GRB 081203B (Copete et al.